The Atmospheres of Venus and MarsJohn C. Brandt, Michael B. McElroy Retells five classic eerie stories in pop-up format, including "Dracula's Guest" and "The Masque of the Red Death." |
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Page 243
... magnetic field will begin to pile up on the windward ( i.e. , the sunward ) side of Mars is given by equating the time for magnetic field lines to be " dragged through " Mars ( or diffuse out of Mars ) with the time for solar wind ...
... magnetic field will begin to pile up on the windward ( i.e. , the sunward ) side of Mars is given by equating the time for magnetic field lines to be " dragged through " Mars ( or diffuse out of Mars ) with the time for solar wind ...
Page 244
... magnetic field near the surface of the cube to the current flowing within it . Thus , from B⚫ dl = μoJ , IB , ≈ μ。J , ( 4 ) where B , is the magnetic field due to the current flowing through the cube . We are interested in the ...
... magnetic field near the surface of the cube to the current flowing within it . Thus , from B⚫ dl = μoJ , IB , ≈ μ。J , ( 4 ) where B , is the magnetic field due to the current flowing through the cube . We are interested in the ...
Page 248
... field lines diffuse through the Martian ionosphere . However , at certain local times , the plasma has direct ac- cess to the upper atmosphere along magnetic field lines ( in Figure 2 SOLAR WIND INTERPLANETARY MAGNETIC FIELD LINES SHOCK ...
... field lines diffuse through the Martian ionosphere . However , at certain local times , the plasma has direct ac- cess to the upper atmosphere along magnetic field lines ( in Figure 2 SOLAR WIND INTERPLANETARY MAGNETIC FIELD LINES SHOCK ...
Contents
Preface | 1 |
Introductory Comments on Venuss Lower Atmosphere | 15 |
Multiple Light Scattering in Planetary Atmospheres | 35 |
Copyright | |
9 other sections not shown
Common terms and phrases
absorption albedo altitude angle atmos atmosphere of Mars band Belton Brandt/McElroy BRAZZA calculated Chamberlain and McElroy cloud cm³ sec-1 CO₂ coefficient computations cross-sections curve diffusion Earth effect electron density energy loss equation Eshleman estimates excitation exospheric exospheric temperature F₁ F₂ Figure Fjeldbo flux G. P. Kuiper Geophys Goody heat Hunten infrared ionization ionosphere isotropic JUIN Kitt Peak Kliore Kuiper layer loss rate lower atmosphere magnetic field magnetosheath Mariner Martian atmosphere Martian ionosphere Martian upper atmosphere measurements mesopause method N.MEXICO N₂ neutral number density observed obtained occultation optical optical depth optical thickness particles peak phase function photoelectrons planet planetary plasma scale pure CO2 radiation radiative Rasool reaction recombination refractivity region rotation scale height scattering solar wind Space Sci spectra spectrum Spinrad surface pressure thermal thermopause thermosphere thick tion vertical water vapor wave wavelength